Searching for planets around eclipsing binary stars using timing method: NSVS 14256825
330th Symposium of the International-Astronomical-Union (IAU), Nice, Fransa, 24 - 28 Nisan 2017, cilt.12, ss.405-406, (Tam Metin Bildiri)
- Yayın Türü: Bildiri / Tam Metin Bildiri
- Cilt numarası: 12
- Doi Numarası: 10.1017/s1743921317005658
- Basıldığı Şehir: Nice
- Basıldığı Ülke: Fransa
- Sayfa Sayıları: ss.405-406
- Atatürk Üniversitesi Adresli: Evet
Özet
We present four new mid eclipse times and an updated O-C diagram of the short period eclipsing binary NSVS14256825. The new data follow the (O-C) trend and its model proposed in Nasiroglu et al. (2017). The (O-C) diagram shows quasi-periodic variations that can be explained with the presence of a brown-dwarf in a quasi-circular circumbinary orbit.